Galileo's Telescope
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Galileo and the Telescope
Galileo and the Telescope A Discussion of Galileo Galilei and the Beginning of Modern Observational Astronomy ___________________________ Billy Teets, Ph.D. Acting Director and Outreach Astronomer, Vanderbilt University Dyer Observatory Tuesday, October 20, 2020 Image Credit: Giuseppe Bertini General Outline • Telescopes/Galileo’s Telescopes • Observations of the Moon • Observations of Jupiter • Observations of Other Planets • The Milky Way • Sunspots Brief History of the Telescope – Hans Lippershey • Dutch Spectacle Maker • Invention credited to Hans Lippershey (c. 1608 - refracting telescope) • Late 1608 – Dutch gov’t: “ a device by means of which all things at a very great distance can be seen as if they were nearby” • Is said he observed two children playing with lenses • Patent not awarded Image Source: Wikipedia Galileo and the Telescope • Created his own – 3x magnification. • Similar to what was peddled in Europe. • Learned magnification depended on the ratio of lens focal lengths. • Had to learn to grind his own lenses. Image Source: Britannica.com Image Source: Wikipedia Refracting Telescopes Bend Light Refracting Telescopes Chromatic Aberration Chromatic aberration limits ability to distinguish details Dealing with Chromatic Aberration - Stop Down Aperture Galileo used cardboard rings to limit aperture – Results were dimmer views but less chromatic aberration Galileo and the Telescope • Created his own (3x, 8-9x, 20x, etc.) • Noted by many for its military advantages August 1609 Galileo and the Telescope • First observed the -
Practical Calculations for Designing a Newtonian Telescope
Practical Calculations for Designing a Newtonian Telescope Jeff Beish (Rev. 07 February 2019) INTRODUCTION A Newtonian reflecting telescope can be designed to perform more efficiently than any other type of optical system, if one is careful to follow the laws of nature. One must have optics made from precision Pyrex or a similar material and figured to a high quality. The mounting hardware must be well planned out and properly constructed using highest quality materials. The Newtonian can be used for visual or photographic work, for "deep sky" or "planetary" observing, or a combination of all these. They are easy to layout and to construct using simple household tools. The design mathematics is simple and can be easily accomplished by hand calculator. The Newtonian reflector can be easily modified for other types of observing such a photometry, photography, CCD imaging, micrometer work, and more. Since a reflecting telescope does not suffer for chromatic aberration we don't have to worry about focusing each color while observing or photographing with filters as we would in a single or double lens refractor. This is a problem especially associated with photography. Since the introduction of the relatively low cost Apochromatic refractors (APO) in the past few years these problems no longer hamper the astrophotographer as much. However, the cost of large APO's for those requiring large apertures is prohibitive to most of us who require instruments above 12 or so inches. Remember, even with the highest quality optics a Newtonian can be rendered nearly useless by tube currents, misaligned components, mirror stain, and a secondary mirror too large for the application of the instrument. -
Galileo Galilei Introduction Galileo Galilei (1564–1642) Was One of The
Galileo Galilei Introduction Galileo Galilei (1564–1642) was one of the most significant figures of the Scientific Revolution. Galileo was involved in nearly all fields of natural philosophy, including astronomy, mathematics, and what we now term “physics.” He is rightly considered one of the founders of modern physics and astronomy, and one of the main originators of the modern scientific method. Galileo’s study of motion became the foundation for Newton’s laws of motion and the principles of inertia and gravity. His astronomical studies were instrumental in supporting the heliocentric model of the solar system first propounded by Copernicus. He should also be credited with making experimentation the basis of scientific study, and with the use of mathematics as the fundamental means for expressing and validating the findings of experimental investigation. Galileo’s application of mathematics to experimental results has become one of the most important aspects of modern science. Galileo made important improvements to the telescope, which enabled him to make great advances in astronomical observation. His observations emboldened him to become the most important advocate of Copernicanism—the astronomical system created by Nicolaus Copernicus (1473–1543)—and his support ultimately ushered in the Copernican revolution in astronomy. Copernicus had devised a heliocentric model in which he posited that the Earth revolved around the sun (in perfect circles). Contrary to the Ptolemaic system and Christian cosmology, Copernicus positioned the sun as a fixed center around which Mercury, Venus, Earth, Mars, Jupiter, and Saturn orbited. Furthermore, Copernicus posited the diurnal rotation of the Earth on its own axis in addition to its annual revolutions around the sun. -
The Jesuits and the Galileo Affair Author(S): Nicholas Overgaard Source: Prandium - the Journal of Historical Studies, Vol
Early Modern Catholic Defense of Copernicanism: The Jesuits and the Galileo Affair Author(s): Nicholas Overgaard Source: Prandium - The Journal of Historical Studies, Vol. 2, No. 1 (Spring, 2013), pp. 29-36 Published by: The Department of Historical Studies, University of Toronto Mississauga Stable URL: http://jps.library.utoronto.ca/index.php/prandium/article/view/19654 Prandium: The Journal of Historical Studies Vol. 2, No. 1, (2013) Early Modern Catholic Defense of Copernicanism: The Jesuits and the Galileo Affair Nicholas Overgaard “Obedience should be blind and prompt,” Ignatius of Loyola reminded his Jesuit brothers a decade after their founding in 1540.1 By the turn of the seventeenth century, the incumbent Superior General Claudio Aquaviva had reiterated Loyola’s expectation of “blind obedience,” with specific regard to Jesuit support for the Catholic Church during the Galileo Affair.2 Interpreting the relationship between the Jesuits and Copernicans like Galileo Galilei through the frame of “blind obedience” reaffirms the conservative image of the Catholic Church – to which the Jesuits owed such obedience – as committed to its medieval traditions. In opposition to this perspective, I will argue that the Jesuits involved in the Galileo Affair3 represent the progressive ideas of the Church in the early seventeenth century. To prove this, I will argue that although the Jesuits rejected the epistemological claims of Copernicanism, they found it beneficial in its practical applications. The desire to solidify their status as the intellectual elites of the Church caused the Jesuits to reject Copernicanism in public. However, they promoted an intellectual environment in which Copernican studies – particularly those of Galileo – could develop with minimal opposition, theological or otherwise. -
Galileo and Bellarmine
The Inspiration of Astronomical Phenomena VI ASP Conference Series, Vol. 441 Enrico Maria Corsini, ed. c 2011 Astronomical Society of the Pacific Galileo and Bellarmine George V. Coyne, S.J. Vatican Observatory, Vatican City State Abstract. This paper aims to delineate two of the many tensions which bring to light the contrasting views of Galileo Galilei and of Cardinal Robert Bellarmine with respect to the Copernican-Ptolemaic controversies of the 16th and 17th centuries: their respective positions on Aristotle’s natural philosophy and on the interpretation of Sa- cred Scripture. Galileo’s telescopic observations, reported in his Sidereus Nuncius, were bringing about the collapse of Aristotle’s natural philosophy and he taught that there was no science in Scripture. 1. Introduction This paper investigates the tensions between two of the principal protagonists in the controversies involved in the birth of modern science, Galileo Galilei and Cardinal Robert Bellarmine, and how they were resolved or not in a spirit of accommodation. Bellarmine’s fellow Jesuits at the Roman College confirmed Galileo’s Earth-shaking observations, reported in his Sidereus Nuncius. Aristotle’s physics was crumbling. Would Aristotelian philosophy, which was at the service of theology, also collapse? Controversies over the nature of sunspots and of comets seemed to hold implications for the very foundations of Christian belief. Some Churchmen saw the threat and faced it with an astute view into the future; others, though pioneers as scientists, could not face the larger implications of the scientific revolution to which they with Galileo con- tributed. Much of what occurred can be attributed to the strong personalities of the individual antagonists and Bellarmine will prove to be one of the most important of those personages. -
Galileo's Assayer
University of Nevada, Reno Galileo's Assayer: Sense and Reason in the Epistemic Balance A thesis submitted in partial fulfillment of the requirements for the degree of Master of Arts in History. by James A Smith Dr. Bruce Moran/Thesis Advisor May 2018 c by James A Smith 2018 All Rights Reserved THE GRADUATE SCHOOL We recommend that the thesis prepared under our supervision by JAMES A. SMITH entitled Galileo's Assayer: Sense and Reason in the Epistemic Balance be accepted in partial fulfillment of the requirements for the degree of MASTER OF ARTS Bruce Moran, Ph.D., Advisor Edward Schoolman, Ph.D., Committee Member Carlos Mariscal, Ph.D., Committee Member Stanislav Jabuka, Ph.D., Graduate School Representative David W. Zeh, Ph.D., Dean, Graduate School May, 2018 i Abstract Galileo's The Assayer, published in 1623, represents a turning point in Galileo's philo- sophical work. A highly polemical \scientific manifesto," The Assayer was written after his astronomical discoveries of the moons of Jupiter and sunspots on a rotating sun, but before his mature Copernican work on the chief world systems (Ptolemaic versus Copernican). The Assayer included major claims regarding the place of math- ematics in natural philosophy and how the objects of the world and their properties can be known. It's in The Assayer that Galileo wades into the discussion about the ultimate constituents of matter and light, namely, unobservable particles and atoms. Galileo stressed the equal roles that the senses and reason served in the discovery of knowledge, in contradistinction to Aristotelian authoritarian dogma that he found to hinder the processes of discovery and knowledge acquisition. -
Autobiography of Sir George Biddell Airy by George Biddell Airy 1
Autobiography of Sir George Biddell Airy by George Biddell Airy 1 CHAPTER I. CHAPTER II. CHAPTER III. CHAPTER IV. CHAPTER V. CHAPTER VI. CHAPTER VII. CHAPTER VIII. CHAPTER IX. CHAPTER X. CHAPTER I. CHAPTER II. CHAPTER III. CHAPTER IV. CHAPTER V. CHAPTER VI. CHAPTER VII. CHAPTER VIII. CHAPTER IX. CHAPTER X. Autobiography of Sir George Biddell Airy by George Biddell Airy The Project Gutenberg EBook of Autobiography of Sir George Biddell Airy by George Biddell Airy This eBook is for the use of anyone anywhere at no cost and with almost no restrictions whatsoever. You may copy it, give it away or re-use it under the terms of the Project Gutenberg Autobiography of Sir George Biddell Airy by George Biddell Airy 2 License included with this eBook or online at www.gutenberg.net Title: Autobiography of Sir George Biddell Airy Author: George Biddell Airy Release Date: January 9, 2004 [EBook #10655] Language: English Character set encoding: ISO-8859-1 *** START OF THIS PROJECT GUTENBERG EBOOK SIR GEORGE AIRY *** Produced by Joseph Myers and PG Distributed Proofreaders AUTOBIOGRAPHY OF SIR GEORGE BIDDELL AIRY, K.C.B., M.A., LL.D., D.C.L., F.R.S., F.R.A.S., HONORARY FELLOW OF TRINITY COLLEGE, CAMBRIDGE, ASTRONOMER ROYAL FROM 1836 TO 1881. EDITED BY WILFRID AIRY, B.A., M.Inst.C.E. 1896 PREFACE. The life of Airy was essentially that of a hard-working, business man, and differed from that of other hard-working people only in the quality and variety of his work. It was not an exciting life, but it was full of interest, and his work brought him into close relations with many scientific men, and with many men high in the State. -
Telescopes and Binoculars
Continuing Education Course Approved by the American Board of Opticianry Telescopes and Binoculars National Academy of Opticianry 8401 Corporate Drive #605 Landover, MD 20785 800-229-4828 phone 301-577-3880 fax www.nao.org Copyright© 2015 by the National Academy of Opticianry. All rights reserved. No part of this text may be reproduced without permission in writing from the publisher. 2 National Academy of Opticianry PREFACE: This continuing education course was prepared under the auspices of the National Academy of Opticianry and is designed to be convenient, cost effective and practical for the Optician. The skills and knowledge required to practice the profession of Opticianry will continue to change in the future as advances in technology are applied to the eye care specialty. Higher rates of obsolescence will result in an increased tempo of change as well as knowledge to meet these changes. The National Academy of Opticianry recognizes the need to provide a Continuing Education Program for all Opticians. This course has been developed as a part of the overall program to enable Opticians to develop and improve their technical knowledge and skills in their chosen profession. The National Academy of Opticianry INSTRUCTIONS: Read and study the material. After you feel that you understand the material thoroughly take the test following the instructions given at the beginning of the test. Upon completion of the test, mail the answer sheet to the National Academy of Opticianry, 8401 Corporate Drive, Suite 605, Landover, Maryland 20785 or fax it to 301-577-3880. Be sure you complete the evaluation form on the answer sheet. -
Revised Final MASTERS THESIS
UNIVERSITY OF CALIFORNIA RIVERSIDE Carlo Fontana and the Origins of the Architectural Monograph A Thesis submitted in partial satisfaction of the requirements for the degree of Master of Arts in Art History by Juliann Rose Walker June 2016 Thesis Committee: Dr. Kristoffer Neville, Chairperson Dr. Jeanette Kohl Dr. Conrad Rudolph Copyright by Juliann Walker 2016 The Thesis of Juliann Rose Walker is approved: Committee Chairperson University of California, Riverside Acknowledgements I would first like to start by thanking my committee members. Thank you to my advisor, Kristoffer Neville, who has worked with me for almost four years now as both an undergrad and graduate student; this project was possible because of you. To Jeanette Kohl, who was integral in helping me to outline and finish my first chapter, which made the rest of my thesis writing much easier in comparison. Your constructive comments were instrumental to the clarity and depth of my research, so thank you. And thank you to Conrad Rudolph, for your stern, yet fair, critiques of my writing, which were an invaluable reminder that you can never proofread enough. A special thank you to Malcolm Baker, who offered so much of his time and energy to me in my undergraduate career, and for being a valuable and vast resource of knowledge on early modern European artwork as I researched possible thesis topics. And the warmest of thanks to Alesha Jeanette, who has always left her door open for me to come and talk about anything that was on my mind. I would also like to thank Leigh Gleason at the California Museum of Photography, for giving me the opportunity to intern in collections. -
A New Vision of the Senses in the Work of Galileo Galilei
Perception, 2008, volume 37, pages 1312 ^ 1340 doi:10.1068/p6011 Galileo's eye: A new vision of the senses in the work of Galileo Galilei Marco Piccolino Dipartimento di Biologia, Universita© di Ferrara, I 44100 Ferrara, Italy; e-mail: [email protected] Nicholas J Wade University of Dundee, Dundee DD1 4HN, Scotland, UK Received 4 December 2007 Abstract. Reflections on the senses, and particularly on vision, permeate the writings of Galileo Galilei, one of the main protagonists of the scientific revolution. This aspect of his work has received scant attention by historians, in spite of its importance for his achievements in astron- omy, and also for the significance in the innovative scientific methodology he fostered. Galileo's vision pursued a different path from the main stream of the then contemporary studies in the field; these were concerned with the dioptrics and anatomy of the eye, as elaborated mainly by Johannes Kepler and Christoph Scheiner. Galileo was more concerned with the phenomenology rather than with the mechanisms of the visual process. His general interest in the senses was psychological and philosophical; it reflected the fallacies and limits of the senses and the ways in which scientific knowledge of the world could be gathered from potentially deceptive appearances. Galileo's innovative conception of the relation between the senses and external reality contrasted with the classical tradition dominated by Aristotle; it paved the way for the modern understanding of sensory processing, culminating two centuries later in Johannes Mu« ller's elaboration of the doctrine of specific nerve energies and in Helmholtz's general theory of perception. -
The Evolution of the Early Refractor 1608 - 1683
The Evolution of the Early Refractor 1608 - 1683 Chris Lord Brayebrook Observatory 2012 Summary The optical workings of the refracting telescope were very poorly understood during the period 1608 thru' the early 1640's, even amongst the cogniscenti. Kepler wrote Dioptrice in the late summer of 1610, but it was not published until a year later, and was not widely read or understood. Lens grinding and polishing techniques traditionally used by spectacle makers were inadequate for manufacturing telescope objectives. Following the pioneering optical work of John Burchard von Schyrle, the artisanship of Johannes Wiesel, and the ingenuity of the Huyghens brothers Constantijn and Christiaan, the refracting telescope was improved sufficiently for resolution limited by atmospheric seeing to be obtained. Not until the phenomenon of dispersion was explained by Isaac Newton could the optical error chromatic aberration be understood. Nevertheless Christiaan Huyghens did design an eyepiece which corrected lateral chromatic aberration, although the theory of his eyepiece was not made known until 1667, and particulars published posthumously in 1703. Introduction This purpose of this paper is to draw together the key elements in the development of the early refractor from 1608 until the early 1680's. During this period grinding and polishing methods of object glasses improved, and several different multi-lens eyepiece arrangements were invented. Those curious about the progress of telescope technology during the C17th, be they researchers, collectors, may find this paper useful. The emergence of the refracting telescope in 1608, so simple a device that it could easily be copied, in all likelyhood had its origins almost two decades beforehand. -
Galileo in Early Modern Denmark, 1600-1650
1 Galileo in early modern Denmark, 1600-1650 Helge Kragh Abstract: The scientific revolution in the first half of the seventeenth century, pioneered by figures such as Harvey, Galileo, Gassendi, Kepler and Descartes, was disseminated to the northernmost countries in Europe with considerable delay. In this essay I examine how and when Galileo’s new ideas in physics and astronomy became known in Denmark, and I compare the reception with the one in Sweden. It turns out that Galileo was almost exclusively known for his sensational use of the telescope to unravel the secrets of the heavens, meaning that he was predominantly seen as an astronomical innovator and advocate of the Copernican world system. Danish astronomy at the time was however based on Tycho Brahe’s view of the universe and therefore hostile to Copernican and, by implication, Galilean cosmology. Although Galileo’s telescope attracted much attention, it took about thirty years until a Danish astronomer actually used the instrument for observations. By the 1640s Galileo was generally admired for his astronomical discoveries, but no one in Denmark drew the consequence that the dogma of the central Earth, a fundamental feature of the Tychonian world picture, was therefore incorrect. 1. Introduction In the early 1940s the Swedish scholar Henrik Sandblad (1912-1992), later a professor of history of science and ideas at the University of Gothenburg, published a series of works in which he examined in detail the reception of Copernicanism in Sweden [Sandblad 1943; Sandblad 1944-1945]. Apart from a later summary account [Sandblad 1972], this investigation was published in Swedish and hence not accessible to most readers outside Scandinavia.